based on the PCP13 Planck+highL solutions (i.e., somewhat broader than the dispersion reported in
[1]}). This condition prevents the individual SZ amplitudes from wandering
too far into unphysical regions of parameter space. We apply a
uniform prior of [0,1] on \(\xi ^{\rm tSZ\times CIB}\) . Results from the
complete 2540 \({\rm deg}^2\)  SPT-SZ survey area
[2]} are consistent with Eq. REF 
and, in addition, constrain the correlation parameter to low values,
\(\xi ^{\rm tSZ\times CIB} = 0.113^{+0.057}_{-0.054}\) . The parameter \(\xi ^{\rm tSZ\times CIB}\) 
is not well constrained by the Planck data and so values are sampled by the CamSpec likelihood
that are excluded by
[2]}.
